The formation of charged antimony and bismuth oxide clusters in a pulsed ar
c cluster ion source (PACIS) has been studied with time-of-flight mass spec
trometric techniques. We compare series of antimony and bismuth oxide clust
er anions with their known cationic counterparts. The anionic series (M2O3)
(n)MO2- and (M2O3)(n)O-2(-) have been predicted proceeding from the known c
ationic series (M2O3)(n)MO+ and (M2O3)(n)O+ by adding O2- and have been exp
erimentally established. All these series contain the metal atoms (M=Sb or
Bi) in the formal oxidation state +3. However, only in the case of antimony
, oxygen rich oxide clusters appear, that can be explained with a gradual t
ransition in the oxidation number from +3 to +5 of single antimony atoms in
the cluster. To estimate the influence of the special oxide formation cond
itions comparative investigations with the PACIS and a laser vaporisation c
luster source have been carried out for bismuth oxide cations. The similar
oxide cluster distributions at comparable oxygen availability display clear
ly that the special thermodynamical stability of the discussed magic cluste
rs is the significant driving force for their formation.